AN ABSTRACT OF THE THESES OF Joseph T. Lipka IC Geology for the degree of Master of Science in presented on April 17, 1987 Title: STRATIGRAPHY AND STRUCTURE OF THE SOUTHERN SULPHUR SPRING RANGE, EUREKA COUNTY, NEVADA Abstract approved: Redacted for Privacy G. Johnson U Early Paleozoic limestones and dolomites of the shallow shelf transitional facies belt were mapped in the southern Sulphur Spring Range, Eureka County, Nevada. The four youngest units in the map area are in fault contact with the Lower Devonian rocks and were probably transported westward, along a low-angle normal fault. The minoirlal dolomites of the Hanson Creek Formation, dated as latest Ordovician in the map area, were deposited in a low-energy lagoon. Overlying the Hanson Creek Formation, with a gradational contact, is the lower member of the Lone Mountain Dolomite, a probable reef complex. The exposed thickness of the lower Lone Mountain Dolomite is estimated to be 250 feet. The Lower Devonian Old Whalen Member of the Lone Mountain Dolomite is composed of well-bedded, alternating brown and gray dolomites. The repetition of rock types in the Old Whalen Member indicates recurring shallow marine environments on a broad carbonate platform. The Old Whalen is estimated to be 1400 feet thick. Directly overlying the Old Whalen Member, is the Kobeh Member of the Mc Colley Canyon Formation. Rocks of the Mc Colley Canyon Formation were deposited on a shallow shelf under normal marine conditions. The mid-Lower Devonian Kobeh Member is sparsely to abundantly fosciliferous and varies from a peloidal wackestone to a peloidal sandy wackestone to a sandy peloidal packstone. The thickness is 276 feet. Overlying the Kobeh Member are the abundantly fossiliferous beds of the lower part of the Bartine. Member. The lower part of the Bartine ranges from a wackestone to a packstone and weathers to a chacteristic yellowish tan. The upper part of the Bartine varies from wackestone to packstone, is darker in color, and is sparsely to moderately fcssiliferous. The thickness of the Bartine Member is 189 feet, and it is late Early Devonian in age. The Sadler Ranch Formation is a dolomitic wackestone containing crinoids with or without brachiopods, and it is latest Early Devonian in age. The Sadler Ranch Formation was deposited on a shallow shelf under normal marine conditions. Above the Sadler Ranch Formation is the lower member of the Oxyoke Canyon Sandstone. The lower member of the Oxyoke varies from a peloidal packstone to sandy peloidal wackestone to quartzite. The upper member of the Oxyoke Canyon Sandstone is a structureless dolomitic mixlstone. The Oxyoke Canyon Sandstone was probably deposited in a high to moderate energy lagoon with a subsequent decrease in depositional energy. The Middle Devonian Sentinel Mountain Dolomite overlies the Oxyoke Canyon Sandstone. The Sentinel Mountain is a structureless to finely laminated dolomite that was deposited in a lagoon that initially had open circulation, but which was later cut off. The youngest formation in the map area is the Permian Garden Valley Formation which is a reddish brown silicified conglomerate. The Sadler Ranch Formation, Oxyoke Canyon Sandstone, Sentinel Mountain Dolomite, and Garden Valley Formation are all present as allochthonous blacks, which were transported from the east as a result of movement along low-angle normal faults. The Nooks were juxtaposed on top of the autochthonous Old Whalen Member of the Lone Mountain Dolomite and on the McColley Canyon Formation. Denudation of the Kobeh and Bartine Members of the McColley Canyon Formation occurred as a reguili- of the movement on the faults. The timing of the movement on the low-angle normal faults is Estimated to be Cretaceous because of the eastern source and the pre-Cretaceous age of the allochthonous rocks. The age is still problematical as a consequence of the lack of any cross-cutting dikes or other age-determinable units. Stratigraphy and Structure of the Southern Sulphur Spring Range Eureka County, Nevada by Joseph T. Lip Ica II A THESES submitted to Oregon State University in partial fulfillment of the requirements for the degree of Master of Science Completed April 17, 1987 Commencement June 1987 APPROVED: Redacted for Privacy Pfe4)or of Geoloizain charge of major Redacted for Privacy Departmen Geology Redacted for Privacy Dean of Grad School ( Date thesis is present& Typed by Joseph T. Lipka II April 17, 1987 ACKNOWLEDGEMENTS At the ere of a movie one often sees the credit "...and a cast of thousands". In the case of a thesis, especially this thesis, the more appropriate credit reads "...and a cast of several". I would now like to thank, in writing, those very important "several". Many thanks go to Dr. Johnson, who let me join the team in the middle of the season. Dr. "J" devised the thesis project, are made are (in his unique way) that the project was finished. I wish to thank Lynne Lipka, who also happens to be my wife, for all kinds of stuff. Claudia Regier skillfully picked the conodonts, a thankless task until now. A well thought thank you to the Friday afternoon "T" group, which proved every week that you can get a bunch of geologists together and not once will they even mention geology. Thanks to Mr. Stephen Sans for letting me use his magic machine, without the machine I would still be writing the introduction. A big thank you to my parents, Joseph and Carmen, or as I call them Dad and Mom. I also wish to acknowledge the financial support of Amerada Hess Corporation, Amoco Production Company, Marathon Oil Company, and Mobil Oil Corporation. Last and certainly not least I would like to thank the little fuzzy people, Winky "aunt bubba" and Mauly. TABLE OF CONTENTS INTRODUCTION 1 Purpose 1 Location and description 2 Methods 2 Terminology 5 Previous work 6 Geologic setting 7 HANSON CREEK FORMATION 12 General statement 12 Litho logy and age 13 Contacts and thickness 14 LONE MOUNTAIN DOLOMITE 16 General statement 16 Lone Mountain Dolomite, lower member 17 Lone Mountain Dolomite, Old Whalen Member 20 MCCOLLEY CANYON FORMATION 28 General statement 28 Kobeh Member 29 Bartine Member, lower part 37 Bartine Member, upper part 41 SADLER RANCH FORMATION 44 General statement 44 Litho logy and age 44 OXYOKE CANYON SANDSTONE 48 General statement 48 Oxyoke Canyon Sandstone, lower member 50 Oxyoke Canyon Sandstone, upper member 54 SENTINEL MOUNTAIN DOLOMITE 57 General statement 57 Litho logy and outcrop chacteristics 58 Contacts and age 60 GARDEN VALLEY FORMATION 61 DEPOSITIONAL HISTORY 63 STRUCTURE 73 Cretaceous? low-angle normal faults 73 Tertiary normal faults 80 CONCLUSIONS 81 REFERENCES 84 APPENDIX 88 Faunal lists aryl localities 88 LIST OF FIGURES Figure 1 Page Index map of Nevada, showing counties and area of figure 2. 2 Index map of central Nevada, showing thesis 3 Contact between the brown dolomite and the gray 4 dolomite of the Old Whalen Member of the Lone Mountain Dolomite. Bailey Pass, northern portion of the map area 4 21 Northern boundary of the map area, showing the contact between the Old Whalen Member of the Lone Mountain Dolomite, and the Kobeh Member of the Mc Colley Canyon Formation. 5 27 Typical outcrop of the Kobeh Member of the Mc Colley Canyon Formation. Mulligan Gap area. 30 Figure 6 Page Weathered surface of Kobeh Member wackestone, which contains silicified corals 7 Slabbed sample of wackestone from the Kobeh Member, McColley Canyon Formation. 8 34 Photomicrograph of peloidal sandy wackestone, Kobeh Member of the McColley Canyon Formation. 9 33 36 Hand sample of the brachiopod and trilobite packstone from the lower part of the Bartine Member of the Mc Colley Canyon Formation. 10 Slabbed sample of the crinoidal dolomite from the Saal Pr Ranch Formation. 11 42 45 Outcrop photograph of the lower member of the Oxyoke Canyon Sandstone and the underlying lower part of the Bartine Member of the Mc Colley Canyon Formation. Mulligan Gap area near JL-129. 49 Page Figure 12 Cross-lamination in the lower member of the Oxyoke Canyon Sandstone. 13 Hand sample of the reddish brown silicified conglomerate from the Garden Valley Formation. 14 62 Present juxtaposition of formations in the southern Sulphur Spring Range. 15 51 75 Correlation chart for part of the Lower and Midge Devonian. 76 LIST OF PLATES Plate 1 Geologic Map of the Southern Sulphur Spring Range, Eureka County, Nevada 2 .in pocket Geologic Cram-sections of the Southern Sulphur Spring Range, Eureka County, Nevada .in pocket 3 Mulligan Gap I measured section. .in pocket 4 Mulligan Gap IC measured section. .in pocket STRATLGRAPHY AND STRUCTURE OF THE SOUTHERN SULPHUR SPRING RANGE, EUREKA COUNTY, NEVADA INTRODUCTION Purpose The purpose of this project has been to study, characterize, and map the early Paleozoic rock units in the southern Sulphur Spring Range, Eureka County, Nevada. A second objective was to study the stratigraphy and structure of the rock units and attempt to determine the depositional environments and relationships to the regional paleogeography. A third objective was to obtain conodont and brachiopod data for time correlation of the rock units and to aid in the determination of their depositional environments. 2 Location and Description The map area encompasses the southern quarter of the Sulphur Spring Range. The area is represented on the U.S. Geological Survey Garden Valley 15-minute topographic quadrangle map, which is located approximately 15 'rules northwest of Eureka, Nevada (see Figures 1 and 2). Access to the map area is via unimproved roads which lead off of a county road along the eastern margin of the range. Methods A total of 10 weeks were spent in the field during the fall of 1984 and the summer of 1985. Fieldwork involved mapping Paleozoic units, collecting samples for lithologic and paleontologic study, and measuring and describing sections. Studies of lithology were aided by petrographic examination of representative thin sections. Selected samples were slabbed in order to examine bedding features. Samples ranging from 10 to 20 pounds were collected in the field for the purpose of obtaining conodonts and brachiopods. Conodont 3 HUMBOLDT ELKO Battle 77, --Mountain -4 mil. I ////1 J,* Carlin // PERSHING / LT k? ,..1 t CHURCHILL STOREY Y cf) <4 14 0 A ( \ . 14 Eureka / N ? ) /WHITE PINE / c Area of NJ MINERAL/\ / \ NYE I ESMERELDA 1 1 0 40 80 miles L__ 1 Figure 1. Index map of Nevada. showing counties and area of Figure 2. LINCOLN 4 * Carlin * Battle Mountain 1 ,c' I V 0 -.f I 0 ,.i A? I \ N r=7 I Si L 7 r7-7 if I0 c.. ) 1 a='' al Mill ( 1 rg I 1 Al Cii CI) Si .. fr C/) I .Z4 a.7 E., a, (r 1g i a.e5 g ,' " al :;.-1 n I A 1-1 MOUNTAIN P, 1 * Eureka ( I r.7 (5- I W i 4,'' t: =1, I 0- C.J I I / ce A LONE 1 Thesis U area ci) o I 1 ',' o_ --k-- AI ,' rzi 0 10 imlw \ 20 miles Figure 2. Index map of central Nevada, showing thesis area. 5 samples were prepared by first dissolving the crushed rock material in 10 % formic acid. The insoluhlp residue was then separated in heavy liquid (tetrabromoethane). The conodonts were then hand picked and placed on slides by Claudia Kegler. Dr. Gilbert K]apper, University of Iowa, made the identifications and age determinations of the conodonts. The undissolved residue from the conodont extraction was the primary source for silicified brachiopods. The non-silicified brachiopods were obtained by breaking up the sample in a hydraulic rock-splitter. The cleaned brachiopods were submitted to Dr. J. G. Johnson, Oregon State University, for identification and age determination. A sample of Lower Devonian corals was submitted to Dr. William A. Oliver Jr., U.S. Geological Survey, for identification and age determination. Terminology The carbonate clacification of Dunham (1962) was used for hand sample and thin - section description. Folk's 1965 crystal size designation was used to describe the recrystallized carbonates. The designations are as follows: <0.004 mm aphanocrystalline, 0.004 to 0.016 mm very finely crystalline, 6 0.016 to 0.062 mm finely crystalline, 0.062 to 0.25 mm medium crystalline, 0.25 to 1.0 mm coarsely crystalline, and 1.0 to 4.0 mm is very coarsely crystalline. The same designations were used to describe the sizes of microscopic quartz grains and crinoid columnals present in the thin sections. Rock colors were determined by comparison with the Rock-Color Chart published by the Geological Society of America (1963). Previous Work In the vicinity of the map area, four previous studies have been completed. Carlisle et al. (1957) studied the Devonian stratigraphy in the Sulphur Spring and Pinyon Ranges. Kendall (1975) did an M.S. thesis study of Lower and Middle Devonian strata in the central and northern portions of the Sulphur Spring Range, as part of a county-wide investigation. Colman (1979) studied the petrology and biostratigraphy of the Old Whalen Member of the Lone Mountain Dolomite in the range as a thesis project 7 Geologic Setting At the present-day site of the Great Basin, shallow water sediments were deposited in a westward-thickening wedge from the late Precambrian (approximately 850 Ma.) to the early Paleozoic. This wedge, part of the Cordilleran geosyncline, extended from southern California to the Canadian Arctic (Roberts, 1972) and was the dominant geological feature in eastern, central, and southern Nevada until the middle Paleozoic (Stewart, 1980). In central Nevada, the deposition of shallow water miogeosynclinal sediments, began in the Cambrian, and continued into Ordovician time. Four Ordovician depositional provinces are recognized, from east to west: 1) a carbonate and quartzite province, 2) a shale and limestone province, 3) a shale and chert province, and 4) a chert-shale-quartzite-greenstone province (Stewart, 1980). The Hanson Creek Formation, which in the study area is latest Ordovician and Silurian in age, is within the carbonate and quartzite province. This province is characterized by deposition in lagoons and on shoals (Dunham, 1977; Stewart, 1980). 8 The Silurian was a continuation of the shallow water shelf deposition in the miogeosyncline. This system is the most limited areally and the thinnest of any lower or middle Paleozoic system in Nevada. However, four depositional provinces are recognized, from east to west: 1) a dolomite province, 2) a laminated limestone province, 3) a chert and shale province, and 4) a feldspathic sandstone province (Stewart, 1980). The Lone Mountain Dolomite is within the dolomite province. Rocks in the dolomite province are almost entirely gray, thin- to thick-bedded, with a few dark gray, locally cherty units (Matti and Mckee, 1977; Nichols and Silber ling, 1977; Stewart, 1980). The earlier sedimentary pattern of shallow water deposition in the miogeosynclinal belt to the west, and deeper-water deposition farther west persisted into the Late Devonian. Again, four depositional provinces are recognized: 1) a carbonate and quartzite province, 2) a limestone and shale province, 3) a shale and chert province, and 4) a chert province. Rocks of the southern Sulphur Spring Range are within the carbonate and quartzite as well as the limestone and shale provinces. Those of the carbonate and quartzite province are cliff-forming, thin- to thick-bedded limestones and dolomites, some of which contain quartzose sandy and silty units and 9 interbedded sandstones or quartzites. These units are primarily shallow water subtidal, intertidal, and supratidal sediments formed on a broad inner shelf (Stewart, 1980). The Old Whalen Member of the Lone Mountain Dolomite, the Sadler Ran Ch Formation, the Oxyoke Canyon Formation, and the Sentinel Mountain Dolomite are units exposed in the field area. Collectively, they have depositional characteristics indicative of the carbonate and quartzite province. According to Stewart (1980) rocks of the limestone and shale provinces were deposited in moderately deep water near the outer edge of the shelf. However, depositional textures present in the Kobeh and Bartine Formations of the Sulphur Spring Range indicate a shallow-subtirlal environment of deposition. During the Late Devonian, the pattern of sedimentation changed with the onset of the Antler orogeny. The Late Devonian to Early Mimissippian Antler orogeny produced the Roberts Mountains thrust in which rocks of the deep water siliceous and volcanic assemblages were thrust eastward over shallow water and related rocks. The Sulphur Spring Range lies at the leading or eastern edge of the thrust (Stewart, 1980). The Antler orogeny formed a highland extending from southwestern to northern Nevada and beyond. Detrital material eroded 10 from the Antler belt, formed thick accumulations of sediment during Miszissippian time in an adjacent foreland basin to the east. This pattern of sedimentation, which began in the Mississppian, continued into the Permian. Within Nevada, five major depositional provinces of Permian rocks are recognized. They are from east to west: 1) carbonate, sandstone, and siltstone province in cratonal and rniogeosynclinal areas in eastern Nevada, 2) carbonate-tenigenous detrital province east of the Antler highland, 3) conglomerate and carbonate province within the Antler highland, 4) rocks of an allochthonous, siliceous, and volcanic province within and west of the Antler highland, and 5) volcanic province in westernmcst Nevada. Those of the carbonate- terrigenous province contain abundant silirlagtic detrital material shed eastward from the Antler highland. In the Sulphur Spring Range, the Garden Valley Formation is included in the carbonate-terrigenous detrital province (Stewart, 1980). The Sonoma orogeny took place during Late Permian to the Early Triassic time. This deformation resulted in the eastward movement of ocean-floor sediments over the shallow water deposits of the Antler highland (Stewart, 1980). The Sevier orogeny followed, with deformation beginning in the Early Cretaceous and lasting until Campanian time. Most of Nevada was in the hinterland of the Sevier orogenic belt (Armstrong, 1968). 11 The next major geologic event was defined by crustal extension during the Cenozoic, which produced the present-day block-faulted basins and ranges (Stewart, 1980). 12 HANSON CREEK FORMATION General Statement The oldest unit mapped in the study area is the Ordovician and Silurian Hanson Creek Formation. This formation crops out in the southeastern portion of the map area, on the west side of an east-dipping fault block (see Plate 1). The Hanson Creek Formation was defined by Merriam (1940) along Pete Hanson Creek in the Roberts Mountains. Merriam described the unit as lying between the Eureka Quartzite and a black chert zone. The black chert zone became the base for the Roberts Mountains Formation, which Merriam also described in 1940. Roberts et al.. (1967) described the Hanson Creek Formation as being a dark gray to black, thick-bedded, coarse-grained dolomite which is more thinly bedded toward the top. 13 Litho logy And Age The Hanson Creek Formation, in the southern Sulphur Spring Range, is a finely crystalline dolomite. On weathered surfaces the rocks are a brownish gray where as on fresh surfaces they are dark brownish gray. The unit has undulatory bedding-plane partings at 6 inch to 1 foot intervals. The dolomite is fetid and contains abundant veinlets of calcite. The Hanson Creek Formation is moderately foesW.ferous with silicified crinoids and crinoid fragments being the only macrofossils. The crinoirls are round and very fine- to fine-grained in size. The unit also contains abundant elongate chert nodules, which average three inches in length. In outcrop, the Hanson Creek appears very similar to the Devonian Old Whalen Member of the Lone Mountain Dolomite. However, it is not as well-bedded as the Old Whalen and also contains abundant chert nodules and crinoiris. In thin section, the Hanson Creek Formation is seen to be composed of finely crystalline dolomite; the boundaries of the crystals are well defined. The dolomite is cloudy because of disseminated organic matter, which is present both at grain boundaries and inside the dolomite crystals, Fossil material, primarily crinoid 14 columnals, constitute 10 % of the total rock. Ghosts of crinoid columnals are present and display a sub-parallel alignment. Aside from the sub-parallel alignment of the crinoid ghosts, the rock is homogeneous. Porosity is appoximately 10 % and is present as irregularly shaped vugs or fractures that have been partially infilled with dolomite, or calcite. The Hanson Creek Formation was dated on the basis of conodonts. One sample was assigned to the ordovicius Zone, which is in the uppermost part of the Ordovician (Klapper, written communication, 1985). Elsewhere, the upper Hanson Creek has been dated as early Silurian (Murphy et aL, 1979). Contacts And Thickness The most extensive outcrop of Hanson Creek Formation is found along the west side of an east-dipping fault block. This fault block also contains exposures of the Lone Mountain Dolomite. The contact between the two units is gradational over an interval of approximately 150 feet; from the brownish gray dolomite of the Hanson Creek to the white to light gray of the Lone Mountain Dolomite. The Hanson Creek 15 Formation where faulted, is defined by extensive shearing and the presence of brecciated dolomite and silica coated slickensides. The shearing is most evident in the fault block adjacent to the main Hanson Creek outcrop (see Plate 1). Across the western fault is the down-dropped Old Whalen Member of the Lone Mountain Dolomite. Because the lower contact for the Hanson Creek Formation is not exposed, it was not possible to determine the thickness for the unit. 16 LONE MOUNTAIN DOLOMITE General Statement The Lone Moutain Dolomite was named by Hague in 1892, for exposures at Lone Mountain. The unit was defined as the Paleozoic strata lying between the Eureka Quartzite and the Nevada Limestone. Merriam, in 1940, redefined Hague's Lone Mountain to include only the strata between the Roberts Mountains Formation (described by Merriam in 1940) and the overlying Devonian Nevada Formation. Meniam's (1940) Lone Mountain Dolomite at Lone Mountain is 1570 feet thick. The lower 1170 feet are light gray massive dolomite; the upper 400 feet consist of alternating bands of light and dark dolomite. Nichols and SUberling (1977) divided the Lone Mountain Dolomite into two units in the Roberts Mountains. Colman (1979), in the Sulphur Spring Range, studied the petrology and biostratigraphy of the Old Whalen Member, the uppermost of three informal members of the Lone Mountain Dolomite. Colman divided the 17 Old Whalen Member into two major lithologic groups, each with three subdivisions. The two major lithologic groups are brown dolomite and gray dolomite. As not by Colman, the subdivisions are oonsidered to be representative end members. Of the three subdivisions in the brown and gray dolomite, four were found in the study area. They are: brown peloidal dolomite and brown skeletal fragment dolomite, along with gray laminated dolomite and gray peloidal dolomite. Lone Mountain Dolomite, lower member The lower Lone Mountain Dolomite crops out as a prominent ridge along the southeast flank of the range (see Plate 1). The unit lies in a fault block together with the Hanson Creek Formation. The dolomite is white to light gray to medium light gray on weathered surfaces. Fresh surfaces are light gray to light brownish gray. The Lone Mountain Dolomite, as described by Nichols and Silberling (1977) is a secondary dolomite in which the rock is replaced or further alt -erred after deposition and is generally chacterized by a sugary recrystallized texture. The coarser crystalline Lone Mountain has this sugary texture and nowhere were any primary textures observed. 18 The unit has bedding plane partings spaced 1 to 4 feet. Within the dolomite and throughout the formation are breccia beds which are 1 to 3 feet thick. The breccia has undergone extensive alteration, probably in the telogenic and mesogenic zone, as indicated by the abundant calcite veins, which have destroyed the original fabric of the rock. In thin section, the Lone Mountain Dolomite displays a variance in crystal size from the northern to the southern outcrops. The dolomite in the southern outcrop area tends to be very finely crystalline. In the central and northern parts the crystals range from fine to coarsely crystalline, with medium crystals the most abundant. The coarser crystalline dolomite displays a sharp gradation of crystal sizes. Over an interval of approximately 30 mm, the dolomite changes from fine to medium to coarsely crystalline. The boundaries between the different crystal sizes are sharp. The texture of fine to coarsely crystalline dolomite tends to be equant within each size grouping In two samples a stylolite is present at the boundary. Porosity ranges from 1 to 5% and is in the form of irregularly shaped vugs and fractures. The vugs throughout the unit are infilled with dolomite or calcite. The vugs to the south are infilled with dolomite and chalcedony. In the central and northern 19 areas the vugs are infilled with coarsely crystalline pseudospar or have been enlarged by dissolution. A sample from the north shows a solution breccia. The lower Lone Mountain Dolomite overlies the Hanson Creek Formation with a gradational contact (see Hanson Creek Formation section) over approximately 150 stratigraphic feet. The Lone Mountain is in fault contact with the uppermost member, the Old Whalen, and the Kobeh Member of the Mc Colley Canyon Formation (see Plates 1, and 2). The exposed incomplete thickness of the lower Lone Mountain is estimated to be 250 feet. The age could not be determined in the study area because of a lack of observed fossils. 20 Lone Mountain Dolomite, Old Whalen Member The Old Whalen Member of the Lone Mountain Dolomite is the unit with the greatest areal extent in the map area (see Plate 1). The Old Whalen is composed of alternating, well-bedded, dark brownish gray dolomites and medium gray dolomites. The dark brownish gray dolomite weathers to a brownish gray; the medium gray dolomite weathers to a light gray. The contact between the gray dolomite and brown dolomite tends to be sharp, though some gradation does exist where brown dolomite overlies gray dolomite (see Figure 3). The Old Whalen is a very distinctive unit in the field because of the regular "stair-step" outcrop pattern. The dolomite forms benches which range in thickness from 1 to 6 feet and which are spaced 20 to 60 feet apart. Bedding plane partings occur at 2 to 4 foot intervals. Both the brown and gray dolomite appear blocky in outcrop as the rocks exhibit a columnar-like jointing pattern. Overall, the brown dolomite tends to be finely laminated and fetid while the gray dolomite tends to be structurelem and not fetid. In hand sample, the brown dolomite appears finely laminated, convolute laminated, with some samples containing abundant 21 Figure 3. Contact between the brown dolomite and the gray dolomite of the Old Whalen Member of the Lone Mountain Dolomite. Bailey Pam, northern protion of map area. 22 macrofossiLs. The gray dolomite is finely, and irregularly laminated. The gray dolomite forms the largest outcrops in the map area. The outcrops are cliffs that range from 30 to 60 feet in height. Brecciation is pervasive in the Old Whalen Member. Most brecciation is probably related to faulting because the dolomite appears to be fractured, with the fractures thrilled with calcite. Observed in the vicinity of the breccias are slickensides, some coated with calcite, others with silica. The fault breccias crop out as 1 to 2 foot thick by 10 to 20 foot long "beds" which are perpendicular to strike. An intraformational breccia was found in the northwest portion of the map area. The angular clasts, which range from <1 inch to 3 inches in diameter, are primarily dark brownish gray dolomite; the matrix is composed of medium gray dolomite. In thin section, two types of brown dolomite and two types of gray dolomite are described. 'The brown dolomites are the brown peloidal dolomite and the brown skeletal fragment dolomite. The gray dolomites are the gray laminated dolomite and the gray peLoidal dolomite. The dolomite types are those described by Colman (1979). Two samples of breccia are also described. The brown peloidal dolomite is composed of dolomite crystals 0.016 to 0.062 mm in diameter, or fine to medium crystalline with the 23 average being 0.039 mm. The boundaries of the crystals appear to be slightly leached as the edges of the crystals are irregular or are indistinct. The unit is composed of approximately 80 % dolomite. Organic material is pervasive and gives the crystals a cloudy appearance. Peloirls represent 30% of the rock. The peloids vary from ovoid to elongate pellets which are approximately 0.008 mm in diameter to indeterminate lumps or patch. All of the peloids are evenly distributed. Some of the lumps are ovoid in shape, but are not of a consistent size. Most of the peloids have indistinct boundaries or are themselves indistinct, probably a result of dolomitization. Porosity in the dolomite is in the form of fenestrae, fractures, and irregularly shaped vugs. The pores have been infilled with dolomite crystals which range in size from fine to coarse. The brown skeletal fragment dolomite is composed of dolomite crystals 0.004 to 0.062 mm in diameter with an average of 0.016 mm or finely crystalline. The crystals are equant in texture and the boundaries are slightly leached. The fossil fragments, which compose approximately 40 % of the total rock, are primarily whole or fragmented rugose corals and crinoid fragments in matrix support. The fossil fragments contain medium-sized dolomite crystals (0.25 to 0.062 mm in diameter). The long axes of the fmcils display a subparallel 24 alignment. Porosity is approximately 10 % and is intraparticle (the inside of the corals) or as fractures, both of which are partially infilled with dolomite. The gray laminated dolomite is composed of dolomite crystals <0.004 mm in diameter. The boundaries of the visible dolomite crystals are irregular and extensively leached. Laminations are 1 to 2 mm thick and show significant displacment by fractures. In thin section, the dolomite is seen to be composed of approximately 20% peloids and <5% fossil fragments. The peloids range from 0.004 to 0.016 mm in diameter and are probably pellets which have been subsequently dolomitized. The fossil fragments identified were gastropods and trilobites The dolomite contains a few stylalites. Porosity is 25% and in the form of fractures which have been partially infilled with very fine (0.004 to 0.016 mm in diameter) or coarsely crystalline (0.25 to 1.0 mm) dolomite. The other type of gray dolomite found is a peicidai dolomite. The dolomite contains pellets which range from 0.08 to 0.25 mm and are ovoid to elongate. The pellets compose 10 % of the total rock and are evenly distributed. Pellets in the sample are similar in appearance to the pellets found in the Kcbeh Member of the Mc Colley Canyon Formation. The orientation of the pellets produces a crude 25 lamination. The dolomite is composed of dolomite crystals which range from <0.004 to 0.016 mm in diameter and which are equant. Porosity was estimated to be approximately 20%. The porosity is in the form of fractures and fenestrae, both of which are partially filled with dolomite. The infilling dolomite crystals range from 0.016 to 0.25 mm in diameter. The breccia samples studied are probably intraformational breccias. The clasts are in matrix support. Casts are angular to subrounded and appear to be similar to the dolomites found in the rest of the member. Clact sizes range from 0.008 to 5.0 mm in diameter. The matrix is composed of <0.004 mm dolomite crystals. The clasts are fractured and some contain irregularly shaped vugs. Both the fractures and vugs are infilled with dolomite. The other breccia sample is composed of angular clasts of sandy peloidal packstone to grainstone. The quartz grains are subangular to subrounded, 0.016 to 0.062 mm in diameter, and compose 30 % of the clasts. Another 30% of the clasts are peloids, which are ovoid in shape though some have been squashed. They appear to have been composed of organic and miciitic material, which has subsequently been recrystallized. 26 The lower contact of the Old Whalen Member is covered by undifferentiated Quaternary alluvium. In the southwest portion of the map area, a normal fault separates the Old Whalen from the underlying Lone Mountain Dolomite and Hanson Creek Formation. On the west side of the study area, the Old Whalen is separated from the Permian Garden Valley Formation by a north-south-trending normal fault, which extends the length of the map (see Plate 1). The contact with the overlying Kobeh Member of the McCulley Canyon Formation is sharp (see Figure 4), with an abrupt change in color and outcrop characteristics (see Kobeh Member section). Between the two units, the contact is not observed because of the bench or "stair-step" outcrop pattern of the Old Whalen. The first Kobeh bed is set back from the 'last- Old Whalen bed by 20 to 60 feet, with the interval between the two covered. The lower contact of the Old Whalen is not exposed, but the estimated maximum exposed thickness is approximately 1400 feet. A conodont sample (JL-74) was obtained from the Old Whalen Member in the central portion of the map area. The sample indicates an Early Devonian age (Mapper, written communication, 1985). 27 Figure 4. Northern boundary of the map area, showing the contact between the Old Whalen Member of the Lone Mountain Dolomite (background, right), and the Kobeh Member of the McC alley Canyon Formation (background, left, and foreground). Note that the vegetation limit approximately fnllnws the contact. Also note the bedding of the Old Whalen Member. 28 MCCOLLEY CANYON FORMATION General Statement Overlying the Old Whalen Member of the Lone Mountain Dolomite is the Mc Colley Canyon Formation. The rocks of the Mc Colley Canyon Formation were originally part of the Nevada Limestone of Hague (1883). Merriam (1940) redefined and restricted the Nevada Formation to include the strata above the Lone Mountain Dolomite and below the Devils Gate Limestone. CarliAlp et al. (1957), working in the Sulphur Spring and Pinyon Ranges, subdivided the Nevada Formation into three members. In ascending order they are: the Mc Colley Canyon Member, the Union Mountain Member, and the Tel Canyon Member. Johnson (1962) recognized an abrupt faunal. and Ethological change at the top of the Mc Colley Canyon Member. This break was interpreted to be an unconformity and warranted elevating the McColley Canyon Member to formational status. Gronberg (1967) proposed a three-fold subdivision of the Mc Colley Canyon Formation. In ascending order they are: the Kobeh Member, the Bartine Member, and the Coils Creek Member. 29 Murphy and Gronberg (1970) proposed the three as formal members. In the map area the Mc Colley Canyon Formation is represented by only the Kobeh and Bartine Members. Kobeh Member Directly overlying the Old Whalen Member of the Lone Mountain Dolomite is the Kobeh Member of the Mc Colley Canyon Formation. Rarely was a bed-on-bed contact observed,. because of the "st-air-step" outcrop characteristic of the Old Whalen. The Kobeh Member does not form well - defined "stair-step" bedding like the Old Whalen Member. The Kobeh is only fair to poorly bedded with bedding thickness ranging from 1 to 3 feet (see Figure 5). The poor bedding, limestone lithology, and fossil content of the Kobeh make for a distinct contact. The thickness of the Kobeh, as measured at the Mulligan Gap I section, is 276 feet (see Plate 3). The Kobeh weathers to a medium light gray to light gray, with fresh surfaces a medium gray to brown gray. In hand sample, the Kobeh appears to be a sandy wackestone or packstone; in thin section, the unit is seen to contain abundant peloids as well as sand grains. 30 Figure 5. Typical outcrop of the Robeh Member of the Mc Colley Canyon Formation. Mulligan Gap area. 31' Above the Old Whalen Member, the Kobeh first appears either as a light gray dolomite with sparse orinoicl fragments (see Plate 3) or as a peloidal sandy wackestone. The typical thickness of the dolomite beds is five feet. However, in the southern portion of the map area, the Kobeh has been dolornitized far upsection from the Old Whalen-Kobeh contact. This is probably a secondary dolomitization, perhaps related to hydrothermal activity in the mesogenetic zone (Nichols and Silber ling, 1977). The section of Kobeh that was dolomitized has been repeated by normal faulting; this was discovered by conodont age dating. Above the pPloidal wackestone, the Kcbeh ranges from a peloidal sandy wackestone or packstone to a peloirisl sandy packstone. The Kcbeh Member is sparsely to moderately fossiliferous at the top and base, and moderately to abundantly fossiliferous in the middle. In thin section, the Kobeh Member consists of peloirls which range from 10 to 70% of the total rock. Pe kid sizes range from 0.008 to 0.5 mm in diameter, the average being 0.016 mm. The peloids are elongate to ovoid and are, as a rule, evenly distirbuted throughout the rock. Because of the uniform shape and size of the peloids, they are probably fecal pellets. 32 All of the samples contain quartz grains. Quartz content varies from 5 to 30% of the total rock. The grains are similar to the pellets in size, ranging from 0.008 to 0.5 mm in diameter. They are angular to subrounded and have irregular boundaries indicating leaching. Some of the grains have overgrowths. Fossils and fossil fragments range from 5 to 50% of the allochems. Dimarticulated acinoids as well as fragmented crinoirls are the most abundant fossil type. Fragmented trilobites, brachiopods, rugose corals, bryozoans, gastropods, and mollusks are also found in the unit (see Figure 6, and 7). Asa rule, if only one type of fossil is present it is crinoids, which are generally fragmented. Although ciinoias are the dominant fossil type, in individual samples trilobites, brachiopods, or bryozoans can dominate. In the packstones the long axes of the fossil fragments display a subparallel alignment. In the wackestones the fossils are randomly oriented and distributed. Porosity ranges from <1 to 20% with 5% the average. The porosity is in the form of fractures, some of which have been partially infilled with pseudospar; one sample has the fractures infilled with silica. Samples with corals and bryozoans tend to have intraparticle porosity, infilled with pseudospar or silica. 33 Figure 6. Weathered surface of Kobeh Member wackestone, which contains silicified corals. Note that the corals display a positive relief. 34 Figure 7. Slabbed sample of wackestone from the Kobeh Member, Mc Colley Canyon Formation. and lower right of the sample. Note the large corals in the upper left 35 One sample, a peloidal wackestone from the top of the member, contains mudstone interbeds 2 to 3 mm thick. Organic matter is found primarily in the pellets, which are dispersed throughout the rock. The pellets display varying degrees of compaction; some are flattened, others are elongated. In some samples they are ovoid. In some samples bioturbation appears pervasive, based on the lack of laminae and the even distribution of the peloids. One sample (JL-94) contains vertical burrows filled with micrite, but no pellets or fossil material That sample also displays a fining upward grading of fossil fragments. In JL-116, the pellets define the laminae, which are approximately 2 mm thick. The fossil material has been recrystalli zed to pseudospar or microspar. Sample JL-65, a peloidal packstone, contains a gastropod infilled with micrite, along with trilobite and brachiopod fragments (see Figure 8). The inside of the gastropod contains a few pellets. The age of the Kobeh Member was determined by utilizing both conodonts and brachiopods. The conodonts obtained from the Kobeh range from the ml.catus Zone to the communication, 1985). brachiopod samples kind & Zone (Mapper, written These zones are of mice -Early Devonian age. The belong to the Spinoplmia Zone anterval 5 or 6) and the kobehana Zone anberwa 8 or 9). Both the Spinoplasia Zone and the kobehana Zone fall within the Pragian Stage of the Devonian (Johnson, 1977). Lower 36 L / mm Figure 8. Photomicrograph of peloirial sandy wackestone, Kobeh Member of the Mc Colley Canyon Formation. Note the trilobite fragment in the center of .the photo is within a large gastropod shell, which has been filled with micrite. 37 Bartine Member, lower part Overlying the Kobeh Member are the abundantly fossiliferous beds of the lower part of the Bartine Member. The contact between the two members is obscured at most places by scree from the overlying Oxyoke Canyon Formation. Where the contact is seen it is poorly exposed because of the recessive nature of both the Bartine and Kobeh, but especially the Bartine. The transition from Kobeh to Bartine is characterized by the appearance of yellowish tan soils and abundant silicified brachiopods, some of which have weathered free. The lower Bartine weathers as small plates 3 to 5 inches across and 0.5 to 2 inches thick. The plates vary from the distinctive yellowish tan to various shades of orange. The color of fresh surfaces is medium gray to yellowish gray. Outcrops of the Bartine are found in only one location in the map area, approximately 0.5 miles south of Mulligan Gap. Bedding is very poorly developed, but where seen is 1 to 2.5 feet thick. The thickness of the Bartine, measured at the Mulligan Gap I section, is 183 feet (see Plate 3). This is an estimated thickness because of the lack of outcrops. 38 Even though outcrops are rare, three distinct nth:Logics are evident in the lower Bartine. The are: a sparsely to abundantly fossiliferous (brachiopod) wackestone, a transitional fades, and an abundantly fossiliferous packstone. In hand sample, the wackestone is composed of whale brachiopods which have been aligned so that the long axes parallel the crude bedding. The packstone, in hand specimen, contains abundant brachiopods and trilobites nested to form a fossil hash (see Figure 9). The brachiopods are found whole, disarticulated, and fragmented. The trilobites are found disarticulated or as fragments. The intermediate fades is transitional between the wackestone and the packstone. In thin section, the brachiopod wackestone is seen to be composed of 60% fossil material. Along with the brachiopods, which are whale or disarticulated, the rock contains disarticulated trilobites, whole gastropods, and other mollusks. The fossils display a weak parallel alignment and have been recryst-alli zed to microspar. Porosity is approximately 1% and is in the form of fractures partially infilled with pseudospar. The packstone is seen in thin section to be a sandy peloidal packstone to a peloidal brachiopod wackestone. The peloidal 39 Figure 9. Hand sample of the brachiopod and trilobite packstone of the lower part of the Bartine Member of the Mc Colley Canyon Formation. 40 brachiopod wackestone is composed of 80 % allochems, of which 45% are fossils and 55% are peloids. The fossils are whale brachiopods, disarticulated trilobites, and whale to fragmented gastropods. The fossils display a parallel alignment of the long axes and all are oriented concave down. Showing no alignment, the peloids average 0.008 mm in diameter and are elongate to ovoid. The peloids are uniform in size and shape and are probably fecal pellets. They appear to be completely mientized. Within the fossil layers are very thin micrite beds which contain the pellets. The sample contains what appear to be branching burrows and blebs of micrite with few, if any, pellets. Porosity is very low in the sample (<5%) and is in the form of secondary intraparticle porosity in some of the brachiopods. Fractures present are infilled with pseudospar. The sandy peloidal wackestone is composed of 30 % quartz grains and 50 % all.ochems (the remaining 20 % is micrite), of which 20% is fossil fragments and 80 % is peloids. The quartz grains are angular and average 0.008 mm in diameter, and display undulatory extinction. The peloids also average 0.008 mm in diameter and are elongate to ovoid. pmloitis. Uniform size and shape indicate a fecal pellet origin for the Fossils present in the sample are disarticulated brachiopods and trilobites. Where there are fossil fragments present in the sample there tend to be very few or no quartz grains present. As in the other lower Bartine samples, the sandy pekidal wackstone also 41 displays a parallel orientation of the long axes of fossils. The brachiopods and trilobites have been infilled with authigenic chalcedony. Porosity is approximately 20 % and is in the form of fractures, and irregularly shaped vugs, which are partially infilled with pseudospar. There is some interparticle porosity, which has been infilled with chalcedony. Bartine Member, upper part The upper portion of the Bartine is different from the lower in two aspects. First, the upper unit weathers to a medium light gray with fresh surfaces a medium gray. Second, the upper unit is a sparsely to moderately fossiliferous wackestone overlain by a moderately fossiliferous packstone. Individual beds range from 1 to 3 inches thick. The packstone contains quartz grains and lithoclasts. The fossil material in both lithologies is primarily arinoirls, predominantly represented by doilhip ossicks. The fossils are oriented parallel to the bedding. 42 The succession of lithologies within the upper Bartine is more complex than described above. The wackestone and packstone units are underlain and overlain by thin (1 to 2 inch thick) breccia beds. The breccia beds appear to be composed of wackestone and packstone. The upper packstone is separated from the wackestone by a thin (1 to 2.5 inch thick) mudstone bed. Bedding in the upper unit is fairly well developed compared to the poorly developed bedding in the lower Bartine. The upper unit is exposed at only one location (JL-123), approximately two miles south of Mulligan Gap (see Plate 1). The outcrop is only 6 feet thick and approximately 20 to 30 feet wide, therefore it was not mapped as a separate unit. The upper unit is overlain by the lower unit of the Oxyoke Canyon Formation. A low-angle normal fault delineates the contact. In thin section, the crinoicial wackestone is found to contain c:dnoic3s1 packstone lithoclasts. The rock has a jumbled appearance. The crinoids are disarticulated and are severely leached, some so much that identification is difficult. The crinoids are randomly distributed and oriented. The sample studied is composed of 55% allochems, of which 80 % are crinoids and 20 % are peloids. Some 43 .of the crinoids are of the doithle ossicle variety. The peloids average 0.008 mm in diameter, are ovoid, and completely micritized; they are possibly fecal pellets. The crinoidal packstone lithoclasts are up to 3 mm in diameter and are rounded. The unit contains angular quartz grains similar to those found throughout the area, but they make up only about 1% of the rock. Very little organic matter is present, and that is scattered. Porosity is approximately 10 % and is in the form of fractures and irregularly shaped vugs. The vugs are partially infilled with pseudospar and the fractures are partially infilled with chalcedony. The Bartine Member was age-dated utilizing both conodonts and brachiopods. The conodonts obtained from the Bartine range from the dehiscens Zone to the inversus Zone (Mapper, written communication, 1985). The brachiopods obtained are from the pinyonensis Zone anterval 10 or 11), which is within the Emsian (Johnson, written communication, 1985.). The above data indicate a late Early Devonian age for the Bartine. The conodonts obtained from the upper part (JL-123) are within the inversus Zone (Klapper, written communication, 1985). 44 SADLER RANCH FORMAI:10N General Statement The first of the allochthonous blocks described in the map area is the Sadler Ranch Formation. Kendall (1975) first described the formation, with the type section located west of the Sadler Ranch in the central Sulphur Spring Range. The formation was originally the middle or crinoidal unit of the Union Mountain Member of Carlisle et al. (1957). Kendall (1975) was able to discern three units within the formation: a lower dolomite, a middle crinoidal dolomite, and an upper dolomite. Became the Sadler Ranch Formation occurs as allochthonous blocks in the map area, only an incomplete section was found. The rocks that make up the allochthonous blocks are part of the middle crinoidal dolomite (see Figure 10). Litho logy And Age The Sadler Ranch Formation is light gray to light brownish gray 45 Figure 10. Slabbed sample of the crinoidal dolomite from the Sadler Ranch Formation. Note the double ossicle crinoiris in the upper left and center of the sample 46 on weathered surfaces. gray. Fresh surfaces are medium gray to brownish The lithology varies from a dolomitic crinaidal wackestone to a dolomitic crinoid-brachiopod wackestone. The dolomitic crinnirlal-brachiopod wackestone alternates with two inch thick, well-bedded dolomitic mudstone and dolomitic silty mudstone. There is also a dolomitic ccinoirlal packstone. The contacts between the units are sharp and undulatory. All the dolomites are fetid on a fresh break. Bedding plane partings occur at one to six foot intervals. The crinoids and the other fossil fragments are calcareous and in some beds display a subparallel orientation. Most of the crinoids are very distinct because they have doithlP cesicles. The double-ossicle crinaids are found in only one other unit, the upper part of the Bartine Member. The Sadler Ranch Formation samples studied in thin section are of the dolomitic crinoirlal wackestone. The unit contains approximately 30 % cclumnals, which are composed of calcite. The crinoirls are randomly distributed and oriented throughout the sample. Approximately 20 % of the total rock is composed of angular to subrounded, very fine-grained quartz. The dolomite crystals range from aphanocrystalline to finely crystalline. is estimated to be 80 %. The amount of dolomite The crystals have irregular boundaries and are cloudy; most are leached. 47 The conodonts which date the Sadler Ranch Formation range from the serotinus Zone to the patiilns Zone (Klapper, written communication, 1985). Devonian. This places the formation in the late Early The age determination in the map area for the Sad Pr Ranch Formation correlates with the conodont--baesd dates obtained by Kendall et at (1983). 48 OXYOKE CANYON SANDSTONE General Statement The Oxyoke Canyon Sandstone is one of the five units that Nolan et al_ defined in 1956. They described it as composed of fine- to medium-grained, rounded quartz in a dolomitic matrix. They also reported that where faulting had occurred the Oxyoke Canyon Sandstone became vitreous and quartzitic. Hose et al. (1982) raised the Oxyoke Canyon Sandstone to formational status. The Oxyoke Canyon Sandstone variously overlies the Bartine (see Figure 11) and Kobeh members of the McCulley Canyon Formation, and the Old Whalen Member of the Lone Mountain Dolomite (see Plate 2). The contact is a low-angle normal fault and is obscured at most places by scree from the very resistant Oxyoke Canyon Sandstone. The most visible contact is the sharp Oxyoke Canyon-Kobeh contact. The upper unit of the Oxyoke Canyon Sandstone overlies the lower unit of the Oxyoke with a gradational contact over an interval of tens of feet, in the southern map area. The Sentinel Mountain Dolomite overlies only the lower unit of the Oxyoke Canyon Formation (see Plate 2, section A -A). 49 Figure 11. Outcrop photograph of the lower member of the Oxyoke Canyon Sandstone (background) and the underlying lower part of the Bartine Member of the Mc Colley Canyon Formation (foreground). Note that the hat is resting on the top of the Bartine Member bed. Mulligan Gap area, near JL-129. 50 The Oxyoke Canyon Formation and the Sentinel Mountain Dolomite are both allochthonous units which were brought into the area by movement along low-angle normal faults. A low-angle normal fault separates the Oxyoke Canyon from the overlying Sentinel Mountain Dolomite. In the central map area the upper unit is separated from the lower unit by a 6 inch chert bed. This is probably a fault plane. Oxyoke Canyon Sandstone, lower member The lower Oxyoke in hand specimen appears to be a very fine- to medium-grained, moderately well sorted sandstone with subrounded to rounded grains. However, in thin section the composition of the lower part of the Oxyoke Canyon is not so simple. The lower unit in the Oxyoke Canyon Formation varies from a peloidal packstone to a sandy peloidal wackestone, both of which have been dolomitized, to a quartzite. The color on fresh surfaces is white to light gray. Weathered surfaces are light red, light brown, medium gray, or light brownish gray. The lower Oxyoke is commonly iron-stained. Finely laminated at the base, the member becomes cross-laminated upsection (see Figure 51 Figure 12. Cross-lamination in the lower member of the Oxyoke Canyon Sandstone. 52 12), and then again finely laminated. The sets of the cross strata range from three to twelve inches thick. The lower Oxyoke Canyon crops out as cliffs from five to one hundred feet high. The lower unit is best exposed in the Mulligan Gap area and just south of JL-123. The lower Oxyoke Canyon is probably the most resistant unit in the study area. This is exemplified by the presence of the unit on the tops of the hills where it acts as a cap, protecting the less resistant units below, i.e. the Bartine and Kobeh Members. Also, many small landslide blocks of the lower unit are seen down slope from the main outcrops (see Plate 1). Because the lower unit is so resistant the underlying units tend to be buried by the scree derived from the lower Oxyoke. Most Bartine Member exposures are completely covered by the scree. A sample of the lower unit was dated with conodonts. The sample yielded Icriodus sp. indef.. (Klapper, written communication, 1985) which indicates a Devonian age for the unit. The significance of the Devonian age is that on lithologic criteria the lower Oxyoke, especially the quartzite at the top of the range, can be confused with the Eureka Quartzite, which is widespread throughout the county. In thin section, the peloidal packstone is seen to be composed almost entirely of pellets; 90 % of the allochems are pellets and 90 % of the rock is made up of allochems. There is some fossil material 53 present that is identifiable as fragmented crinoids. In addition, 1% of the rock is angular, very fine quartz. The matrix has been dolomitized, with the crystals ranging from <0.004 to 0.016 mm in diameter. The peloids, which average 0.008 mm in diameter and are elongate to ovoid, probably are fecal pellets which have been completely micritized. mm thick. The unit is laminated with laminae one to two The crinoirls and the other fossil material have the long axes oriented parallel to the laminae. Interparticle porosity and irregularly shaped vugs make up the 5% porosity found in the sample. In thin section, the sandy peloidal wackestone is composed of 40 % quartz grains and 10 % peloids. The quartz grains are subrounded to rounded, very well sorted, and average 0.008 mm in diameter. The matrix has been dolomitized with the crystals medium to coarse in size. The quartz grains all exhibit undulatory extinction. The peloids, probably pellets, average 0.008 mm in diameter and are evenly distributed throughout the sample. The pellets are ovoid, though some are squashed and appear to have been completely micritized. There are larger peloids composed of several pellets squashed together. Porosity is <5% and is in the form of void spaces within the matrix. 54 The other rock type in the lower Oxyoke Canyon Sandstone is a quartzite. In thin section, approximately 30 % of the grains were found to be in optical continuity. The grains range from 0.25 to 0.5 mm in diameter. The grain boundaries are planar with some enfacial triple junctions. Several of the grains were observed to have quartz overgrowths. A few fractures have been infilled with chalcedony. Oxyoke Canyon Sandstone, upper member The upper unit of the Oxyoke Canyon Sandstone is a dolomitic mudstone. The upper unit is best exposed in the Mulligan Gap area; overall, the southern exposures are the most extensive. In the central map area, the upper unit is medium gray on fresh surfaces and light gray where weathered. The dolomite is moderately well-bedded with bedding plane partings approximately one foot apart. In the southern portion of the mapping area the dolomite is brownish gray on fresh surfaces; weathered surfaces are a light brownish gray. The dolomite in the central portion is highly fractured, and in the south the dolomite tends to be.brecciated and fetid. Both the central and southern exposures have quartz-rich dolomite at the base; this dolomite decreases in quartz content upsection. The quartz-rich base 55 is a transitional unit between the sandy peloidal wackesbone-packstone of the lower member and the dolomite of the upper member. The transitional unit is finely laminated, with quartzose layers interbedded with dolomitic mudstone. The quartzose layers are undulatory with some small-scale scour-and-fill structures. In thin section, the transitional unit is seen to be a dolomitized mudstone with undulatory sandy interbeds which range from 2 to 4 mm thick. The quartz grains are very fine- to fine-grained, some are in grain-to-grain contact, and some are in matrix support. The mudstone is very finely laminated. The laminations and the quartzcse interbeds have been disturbed by burrowing organisms. Although the burrows are randomly oriented, most are vertical. The downward displacement of the quartz grains into the mud layers is the most obvious evidence of burrowing. Porosity is <5% and is in the form of fractures. Some of the fractures have produced small-scale normal "faults". These small-scale "faults" resulted in the formation of small-scale grabens of quartzose interbeds. The thin sections of the upper Oxyoke Canyon Sandstone studied were found to be a dolomitic mudstone and a sandy crinoidal dolomite. The dolomitic mudstone is composed of a mosaic of finely crystalline 56 dolomite. Crystal boundaries are irregular and the dolomite is cloudy. Approximately 1% angular very fine-grained quartz is present. Irregularly shaped vugs and fractures make up the estimated 10 % porosity in the rock. The infilling matprial is dolomite, calcite, and chalcedony. The sandy crinoiaal dolomite is composed of 20% quartz grains and 20 % fossil materiAl, All the grains are in matrix support. The quartz grains are angular to subrounded and very fine in size. Some of the grains have coalesced and now display enfacial triple junctions. The crinoid columnals are extremely leached, making identification difficult. The dolomite crystals range from finely to coarsely crystalline, the average size being about 0.8 mm in diameter or coarsely crystalline. In addition, 10% of the rock is estimated to be pore space. The porosity is in the form of vugs partially filled with dolomite and fractures partially filled with chalcedony. 57 SENTLNEL MOUNTAIN DOLOMITE General Statement The Sentinel Mountain Dolomite was originally described as part of a five-fold subdivision of the Nevada Formation by Nolan et al. (1956). They described the Sentinel Mountain as being entirely composed of alternating beds of light and dark dolomite. In 1957, Carlisle et al., in their subdivision of the Nevada Formation in the Sulphur Spring and Pinyon Ranges, described a sequence of alternating beds of light and dark dolomite which they called the Telegraph Canyon Member. Both the Telegraph Canyon and Sentinel Mountain are Middle Devonian. Hose et al. formational status. (1982) raised the Sentinel Mountain Dolomite to Kendall et al. (1983) noted that the lower unit of the Telegraph Canyon Member is correlative with the Sentinel Mountain Dolomite. Johnson and Murphy (1984) proposed a revision of the stratigraphic nomenclature in which they suggested a rejection of duplicate names. The lower unit of the Telegraph Canyon was dropped in favor of the Sentinel Mountain Dolomite as a matter of simple priority. The Sentinel Mountain Dolomite, like the Oxyoke Canyon 58 Sandstone, is an alloctthonous unit, brought into the area as a result of low-angle normal faulting. Litho logy And Outcrop Characteristics In the map area, the Sentinel Mountain occurs as an alternating brownish gray to medium gray, mottled dolomite. The brownish gray dolomite are light brownish gray to light gray. tends to be fetid. The fresh surfaces The unit forms one to six foot thick benches with the benches spaced 10 to 50 feet apart. In the field, the Sentinel Mountain closely resembles the Old Whalen because of similar color and outcrop pattern. The Sentinel Mountain does not contain the gray dolomite of the Old Whalen, however. The lithology of the formation varies from a sandy dolomite at the base to a dolomitic cdrwlicial wackestone and finally to a dolomitic mudstone. The bed is exposed at only two unit there is a localized breccia bed. locations (near JL-54, see Plate 1). At the base of the The breccia consists of angular clasts, from <1 inch to 2 inches across, composed of dolomitized sandy pekAdal wackestone in martiix support. iron-stained. The matrix is heavily 59 The Sentinel Mountain Dolomite in thin section is seen to be a very finely to finely crystalline laminated dolomite. The laminations are <0.25 mm thick. The formation contains only 1% very fine quartz grains, which are extensively leached. One sample contains approximately 5% unident-ifiahlp fine-sized fossil fragments. The long axes of the fossils have a subparallel alignment. The dolomite crystals have a mcsaic texture with fairly straight boundaries. The crystals are cloudy, probably a result of the finely disseminated organic matter. The dolomite contains vertical burrows which disturb the very fine laminations. Because of the homogeneity of the rock, the dolomite was probably a mudstone. The fractures and vugs in the rock have been infilled with dolomite. The breccia unit found near the base of the Sentinel Mountain Dolomite is seen in thin section to be a dalomitized sandy peloidal wackestone breccia. The clasts are subrounded to rounded, and range from 0.008 to 2 mm in diameter. The larger clasts do not contain any peloids; but are a dalomitized sandy wackestone. The dolomite is very fine to medium crystalline. The matrix is extensively leached and iron-stained. The clasts also contain irregular blebs of chalcedony. 60 Contacts And Age The Sentinel Mountain Dolomite is part of the allochthonous package which includes the Sadler Ranch, Oxyoke Canyon Formation, and the Garden Valley Formation. The Sentinel Mountain overlies the Oxyoke Canyon Sandstone with what appears to be a concordant contact. That contact, however, is a low-angle normal fault, with the breccia bed at the base of the Sentinel Mountain possibly marking the trace of the fault that separates the two units. The Sentinel Mountain was dated utilizing conodonts. A sample (JL-54) was obtained approximately 50 stratigraphic feet above the be of the unit. The conodonts found in the dolomite range from the australis Zone to the Lower varcus Subzone (Mapper, written communication, 1985). Middle Devonian. This places the Sentinel Mountain within the 61 GARDEN VALLEY FORMATION The Permian Garden Valley Formation forms a prominent ridge along the western margin of the map area. The Garden Valley Formation was first described by Nolan et al. (1956). The type locality is located approximately two miles south of the study area. At the type locality Nolan et al. (1956) described four members for the Garden Valley. The member which is found in the map area is the reddish brown silicified conglomerate member (see Figure 13). At the type locality the conglomerate is 900 to 1000 feet thick and overlies another silicified conglomerate. The reddish brown conglomerate is composed of angular to subrounded, coarse sand to cobble-sized clasts, which are clastand matrix-supported. The clasts are multi-colored and are composed of microcrystalline quartz. The rock has been thoroughly silicified; in some samples the clasts are merely dark blebs in the matrix. At some outcrops, the conglomerate is darker in color, almost black. Most is reddish brown, which gives the ridge along the western margin of the map area a red color. The eroded material from the formation also has a distinctive red color. The contact between the Garden Valley Formation and the other units is a north-south normal fault which runs the length of the map (see Plate 1). The basal contact of the formation is a low-angle normal fault (see Plate 2) as the Garden Valley is the youngest of the allochthonous rocks in the map area. 62 Figure 13. Hand sample of the reddish brown silicified conglomerate from the Garden Valley Formation. 63 DEPOSITIONAL HISTORY Several rock units were deposited from the latest Ordovician to the Middle Devonian in a shallow sea covering a carbonate shelf at the present-day site of the southern Sulphur Spring Range. During the latest Ordovician, the finely crystalline, dolomitic crinoidal mudstones and wackestones of the Hanson Creek Formation were deposited in a low-energy lagoon. The environment of deposition was determined by Dunham (1977). Dunham studied the Hanson Creek Formation in several areas in Eureka County, but the most applicahlp to this study are the Lone Mountain and Pete Hanson Creek sections; with the latter located in the Roberts Mountains. He concluded that the Hanson Creek was deposited in four distinct environments. The high energy shoals, according to Dunham (1977), dissipated the wave and current energy so that mud-sized material was then deposited in quiet lagoons shoreward of the shoals. The sections at both Lone Mountain and Pete Hanson Creek contain wackestone and mudstone with pelmatazoan columnals. The Pete Hanson Creek section is dominated by mudstone with wackestone interbeds. Dunham (1977) also noted that the fossils present indicate that water circulation must not have been 64 restricted. The fossil content of the Hanson Creek in the southern Sulphur Spring Range is between 5 and 10%, of which all are crinods. Their presence could indicate, as Dunham noted, an unrestricted water circulation, allowing organisms to exist in the lagoon. However, the crinoids found in the map area are disarticulated and do not appear to exceed 2 mm in length. In the case of the southern Sulphur Spring Range these crinoirls were probably washed into the lagoon as the result of storms. The samples studied from the Hanson Creek are not laminated and the crinoids are randomly oriented; therefore, conditions must have been such as to allow burrowing organisms to exist and stir up the substrate. A late Llandoverian hiatus has been documented by Murphy et al. (1979) between the Hanson Creek and the Roberts Mountains Formation. Johnson and Murphy (1984) have projected this unconformity beneath the Lone Mountain Dolomite. Because the Lone Mountain Dolomite is a secondary dolomite, interpretation of the depositional environment is not possible from field or thin section study. However, several authors (Winterer and Murphy, 1960; Math and McKee, 1977; Johnson and Sandberg, 1977; Mullen, 1980) have concluded that the Lone Mountain Dolomite forms a couplet with the Roberts Mountains Formation. The Roberts Mountain 65 Formation is the deeper-water equivalent of the Lone Mountain. Rocks of the Roberts Mountains Formation are basinal limestones and reef flank deposits. The Lone Mountain Dolomite is a reef complex from which the reef flank deposits of the Roberts Mountains were derived. The time of deposition of the couplet was from the late Llandoverian to the Lochkovian (Johnson and Murphy, 1984). A hiatus occurred from the Pridolian to the early Lochkovian (Johnson and Murphy, 1984), after which the upper member, the Old Whalen, of the Lone Mountain Dolomite was deposited during the late Lochkovian (Klapper and Murphy, 1980). The Old Whalen Member represents a variety of repeating rock types, as noted by Colman (1979), that indicates different recurring shallow marine environments on a broad carbonate platform. The brown fetid dolomite represents rapid burial or burial in an oxygen-poor environment, with consequent preservation of the organic matprial, The gray non-fetid dolomite indicates either slower deposition or deposition in oxygenated water where organic matter was destroyed. The presence of peloids in the brown fetid dolomite also indicates anoxic conditions; the few fenestrae present indicate rapid burial, The brown dolomites of the Old Whalen were deposited in areas of quiet water, which were slighty restricted in circulation. The dark color 66 and the fact that the dolomite is fetid would indicate either rapid deposition or deposition under anoxic conditions. However, the presence of pelaids and skeletal material indicate that conditions were probably not anoxic. The lack of abundant fenestrae indicate rapid deposition. Fossils above the substrate, within the dolomite are whale or fragmented rugose corals and crinoids. The presence of crinoirls indicates open marine conditions. The fine crystallinity of the dolomite and the fragmented nature of some of the fossils also implies that the fossils were broken up on a high energy shoal and then washed into a shoreward basin or lagoon. The corals, which are found whole, could have lived along the margins of the basin because the rugose variety can exist on soft substrates. The gray dolomites represent a change in the site of deposition, as they are not fetid. The dolomite, where laminated, is only poorly laminated and contains peloids as well as fragments of gastropods and trilobites. The gray dolomite must have been deposited more slowly than the brown dolomite because the overall massive character of the gray dolomite would indicate bioturbation. Also, the slower rate of deposition may have led to the accumulation of trilobite and gastropod fragments in the gray dolomite versus rugose coral and crinoirls in the brown dolomite. However, the amount of fossil material is more important; in the brown skeletal fragment dolomite up to 50 % of the 67 total rock is allochems, of which 30 % is fossil material. In the gray peloidal dolomite 20% of the total rock is allochems of which <5% is fossil material. The overall lower volume of allochems, especially fossil material, suggests that the amount of material coming from the high-energy shoals was probably less in the gray dolomite. The gray dolomite may represent a period of low-energy deposition; whereas the brown dolomite represents a higher energy deposition on the shoals, which would lead to a greater volume of material coming into the basin during a given period of time. The flood of material causing rapid burial, prevented the substrate from being bioturbated. The cause of the episodic "flooding" of material may have been the result of storms. A major unconformity is present between the Old Whalen Member and the base of the K obeh Member. This unconformity marks the end of the Tippecanoe sequence and the base of the K obeh Member represents the begining of the Kaskaskia sequence (Sloss, 1963; Johnson and Murphy, 1984). 68 Deposition of the Kobeh Member began in the e.arly Pragian. The Kobeh Member was deposited on a shallow shelf under normal marine conditions. The abundant shelly fauna indicates shallow water depths; the crinoids indicate open circulation. Organic activity remained high during deposition as manifested by the presence of peloids throughout the unit. Fossils in the packstones display a subparallel orientation whereas those in the wackestone are randomly oriented. The packstone was deposited or possibly re-worked during storms as evidenced by the subparallel alignment of the fossil fragments and the lack of mud. The wackestones were deposited and then bioturbated as indicated by the lack of laminae and by the random orientation of the fossils. However, bioturbation was not pervasive, as is indicated by the presence of mud interbeds in one peloidal wackestone sample. The sand found throughout the Kobeh could be either ealian or fluvial by transport across the Sevy-Beacon Peak tidal flats. Kendall (1975, Fig. 4) plotted the distribution of a basal quartzite of the Sevy-Beacon Peak Dolomite. The source of the quartzite was to the north and east of the map area, or shoreward of the Kobeh outcrops in the Sulphur Spring Range. Because this sand is present throughout the Kobeh it was probably carried out to the shelf by currents. The currents sorted the sand so that only the finest fraction was deposited off shore. 69 Directly following deposition of the Kobeh was the deposition of the Bartine Member of the Mc Colley Canyon Formation. The initial deposits of the Bartine were laid down in the latest Pragian-earliest Emsian. The Bartine was also deposited in a shallow shelf, normal marine environment, and like the Kcbeh, was affected by variable However, the Bartine appears to be a deeper deposit than currents. the Kcbeh. The Bartine contains more mud than the Kobeh and the fossils in the wackestones are whole or disarticulated, not fragmented as in the Kobeh. The effect of the variable currents or storms caused the fomils in the packstones to be nested, with the brachiopods and trilobites oriented concave down. Additional evidence for the Bartine being farther offshore than the Kobeh is the presence of thin mudstone beds found in between the fossil layers in the packstones. The mud remained because of the diminished effect of currents in the deeper water. The inverse relationship between fossil material and quartz grain content in the packstone is probably storm-related. The stronger currents could have caused both the sand and fossil material to be swept farther out into the basin than usual, but with the fossil material being carried farther offshore than the sand. The peloids and abundant shelly fauna which are found throughout the unit indicate that organic activity was high. Burrows observed in the thin sections indicate that the bottom was not anoxic and that deposition was not 70 sufficiently rapid to prevent bioturbation. The upper part of the Bartine represents further deepening of the basin during the late Emsian. The medium gray color of the upper Bartine versus the yellowish gray of the lower Bartine indicates a deeper water deposition for the upper. Quartz grains compose 1% of the total rock, although in the lower unit, they compose up to 30%. Bedding is better developed in the upper Bartine, and there appears to be no evidence of bioturbation. The lack of shelly fauna would also indicate deeper water than in the lower Bartine. The variable currents were still effective, however, as evidenced by the parallel orientation of the crinoid bedding. The presence of lithoclasts in the packstone indicates that reworking of the substrate occurred. This could have been the result of downslope movement of the substrate or from storm-induced currents reworking the substrate. Crinoids, being the principal fossil, indicate an open marine circulation. The Sadler Ranch Formation was deposited during the late Early Devonian. The dolomitic crinoid, and crinoid-brachiopod wackestones were deposited on a shallow shelf under normal marine conditions. The Shelly fauna indicate shallow water depths and the crinoids indicate open circulation. However, conditions were not stable; as is 71 indicated by the thin mudstone bed and the packstone. The mudstone bed, within the wackestone, suggests an interval of lower depositional energy. The packstone is the result of increased depositional energy with the subsequent winnowing of any mivis that were present. The packstone was probably deposited during or reworked by a storm. The overall. ma give bedding, except in the mudstone bed, indicates bioturbation took place throughout deposition. The very fine grains of quartz found in the Sadler Ranch were probably derived from the beach-bar-dune deposits found in the Oxyoke Canyon Sandstone. The Oxyoke Canyon Sandstone is the shoreward correlative of the Sadler Ranch Formation. The lower member of the Oxyoke Canyon Sandstone was probably deposited in a high to moderate energy lagoon. The lag000n had open circulation as indicated by abundant peloids found throughout the unit. The dolomite matrix indicates a shallow water environment. The pPlnirls show that organic activity was high. The high to moderate depositional energy is indicated by lack of mud, as in the peloidal packstone, and by the croa-laminae in the middle of the unit. The decrease in depositional energy in the lagoon resulted in the deposition of the dolomitic mudstone of the upper member of the Oxyoke Canyon Sandstone. The decrease in energy is suggested by the dolomitic mudstone with quartz interbeds which become dominantly dolomitic mudstone upsection. However, the lagoon retained an opening 72 to the sea as is indicated by the presence of acinoirls. Bioturbation continued throughout deposition; as is documented by the downward displacement of some of the quartz interbeds, and in the overall massive character of the mudstone. The Sentinel Mountain Dolomite was deposited in an environment that was similar to that of the upper member of the Oxyoke Canyon Sandstone; probably in a lagoon that initially had open circulation and that was later, at least partially, isolated from the sea. The sandy dolomite and the dolomitic ctinoidal wackestone were deposited during the time of open circulation. The dolomitic mudstone was deposited during a time of restricted circulation, but not sufficiently restricted as to limit organic activity. The mudstone is dark in color and fetid, but shows evidence of bioturbation. 73 STRUCTURE The prominent structural features in the southern Sulphur Spring Range are a Cretaceous? age low-angle normal (denudation) fault and the steeper more typical normal faults of Tertiary age. The all.ochthonous post-Bartine 6 ata were emplaced by the Cretaceous? low-angle normal fault. The Tertiary normal faults resulted in typical Basin and Range fault-block topography of the area. Cretaceous? Low-angle Normal Faults The low-angle normal faults were discovered by studying the stratigraphic succession, with the aid of paleontological age determinations obtained from the conodonts. The conodonts identified the units more precisely than lithology because of overall lithalogic similarities of some of the units, i.e. the Sentinel Mountain Dolomite and the Old Whalen. The stratigraphic succession was found to vary throughout the map area, with the variance always occurring above the Kobeh Member. The overlying Bartine Member appears to be cut out in 74 places by the lower unit of the Oxyoke Canyon Sandstone (see Figure 14), especially north of the Mulligan Gap area. The stratigraphic succession with low-angle normal faults is illustrated in Figure 14. Stratigraphic relationships between the various rock units would be difficult to explain without the low-angle normal faults. The Bartine Member is incompletely cut out by the shallow water high-energy lower Oxyoke Canyon Sandstone. However, the Bartine has not been removed in the southern map area (JL-123). The present day juxtaposition of the formations (see Figure 14) shows the lower Oxyoke overlying on an almost complete sequence of Bartine, i.e. both the upper and lower parts of the Bartine Member are present. In the central portion of the map area, the Bartine is completely missing, with the Oxyoke Canyon rocks overlying the Kobeh Member. As shown in plate 2 (section A-A'), the lower Oxyoke in the east, is found on the Old Whalen with both the Bartine and Kobeh removed, but not by erosion. Also, in the eastern portion of the map, the Sentinel Mountain Dolomite lies directly on the lower Oxyoke Canyon, whereas the upper Oxyoke is not present. The fades diagram given by Figure 15, shows the lower Oxyoke Canyon as pinching out; the dolomites of the upper Oxyoke Canyon lie on top of the sandstones and pelok1al packstones of the lower Oxyoke. o 0-..t. South North Low-angle normal fault --MWM--AMn nippy JL-123 1 ,---- Doxu -1-, 0 0 , cl-1 1 4-1 M M rr Doxl Dmb 0 .1-1 El Dmk o ,---"""--",-/1,----",/"W-...-----,...-----,----Nz------,.....- __,".,/--s./'' . 1 Dirnow Figure 14. Present juxtaposition of formations in the southern Sulphur Spring Range. Facie:: Plnco Lone Mountain Southern Sulphur spring Range 1 Source, Kendall et ni., 1903 I 2 Sulphur Kendall et al., 1983 Sentinel Mtn. Dolomite Sentinel Mtn. Dolomtte In the Southern Sulphur Spring Range, otratigraphic sections 1, 2, and 3, are locatod near the following fosuil locolitleo (see Plate 1): Diamond Range Spring Ron.g2 3 Thin Paper Denny Limontono 1 I EXPLANATION Transitional & Lau tern TrannitIonal Wel:tern Belt Nolan et al. 1956 Sentinel Mm. 2 Mbr. 0 11111-111111-1110L- t- I w upper Member m vi 11 Black rectangles denote horizono affected by low-angle normal faulting. Oxyoke Canyon Po/Illation If Z1 Oxyoke Canyon Sadler Ranch Formation Mbr. Oxyokc Canyon Sandstone lower member -1211-11111-11:21-1Cla _ONLABIL Sadler Ranch Fm. Sadler Rancl Fm. moo is jra o 111 rrt uppe Coils Creek Bartine Tongue Mbr. ..4 , ] 3 JL-119 JL-54 JL-123 g p w 3. o 14 14 o ... Datine Mbr. Bartino Beacon Peak U. Tongue Mbr. Bartino lower part Koboh Koboh Kobeh Kobel: Mbr. Mbr. Mbr. Mbr. w H H 00 Lone Mtn. Dolomite Figure15. Old Ullle Member Beacon Peak br. Bartino Mbr. Mr. >,. Deacon Peak Dolomite Lone Mountain Dolomite Correlation chart for part of the Lower and Middle Devonian. 77 As shown in the correlation chart (see Figure 15), the stratigraphy in the southern Sulphur Spring Range is not totally compatible with that in other areas of the county. Kendall (1975) has demonstrated that the Sadler Ranch Formation overlies the Bartine Tongue in the central and northern portions of the Sulphur Spring Range. The Sadler Ranch is, in turn, directly overlain by the Oxyoke Canyon Formation. To the south of the Sulphur Spring Range, at Lone Mountain, the Sadler Ranch Formation is underlain by the Coils Creek Member of the Mc Colley Canyon Formation, and is overlain by the Denay Limestone. East of the Sulphur Spring Range, in the Diamond Range, the Oxyoke Canyon is underlain by the Beacon Peak, and is overlain by the Sentinel Mountain Dolomite. Elsewhere there are units missing from the normal stratigraphic succession in the southern Sulphur Spring Range (see Figure 15); i.e. the Oxyoke Canyon Sandstone lies directly on Bartine Member with no Sadler Ranch present, and the Sentinel Mountain Dolomite overlies the lower member of the Oxyoke Canyon with the upper portion of the Oxyoke Canyon missing (location 2, Figure 15). Also at location 2, the Sadler Ranch Formation lies directly upon the Old Whalen Member with the Mc Colley Canyon rocks missing The Sadler Ranch Formation, Oxyoke Canyon Formation, and Sentinel Mountain Dolomite display a complicated relationship with other rock 78 units in the area. Explanation for these relationships using fades changes would require anomalous changes in the depositional environment, that would not be in agreement with W alther's laws of fades. The simplest solution to these stratigraphic problems is obtained from structural investigations. Low-angle normal faults are commonly characterized by the juxtaposition of younger strata over older, with the removal of strata, or denudation, at horizons affected by the faults. The southern Sulphur Spring Range is a prime example of this phenomenon. The Lower to Middle Devonian Oxyoke Canyon Sandstone, along with the Sadler Ranch Formation and the Sentinel Mountain Dolomite, have been juxtaposed on the Lower Devonian Old Whalen, Kobeh, and Bartine Members. The incomplete removal of the Bartine Member and the complete removal of the post-Bartine units also took place (see Figures 14 and 15). The solution to the succession problem is believed to be in the low-angle normal faults. Low-angle normal or denudation faults have been studied in eastern Nevada by Armstrong (1972) and other workers (Coney, 1974; Hose and Blake, 1976). Low-angle faults are the product of extension, and, in the case of the southern Sulphur Spring Range, were probably related to the Cretaceous Sevier orogeny. There has been disagreement among the various investigators as to the timing of the low-angle faulting. For example, was the movement a Cretaceous or a Tertiary event? The answer cannot be found in the southern Sulphur Spring Range because of the lack of any cross-cutting dikes or other 79 age-determinable units. A Cretaceous age of movement on the low-angle fault in the southern Sulphur Spring Range is presumed because of the eastern source and the pre-Cretaceous age of the allochthonous rocks. The age is still problematical as a consequence of the lack of evidence for the time of movement. Johnson (1986, written corn mmunication) has stated that the source of the allochthonous rocks was to the east because there is not an example in estahlished stratigraphy of Oxyoke Canyon over a full develpoment of Bartine, as is juxtaposed in the southern Sulphur Spring Range. The Oxyoke Canyon Sandstone and the remainder of the allochtonous package, therefore, must have come from the east. As indicated on the A-A' cross- section in Plate 2, the Garden Valley Formation is also part of the allochthonous package. This is in agreement with drill data (J. P. Graham, 1986, written communication) showing that four wells drilled in Diamond Valley ( T 23N-R 54E-NE NW 30, T 24N-R 53E-NW NW 24, T 21N-R 53E-NE NW 1, and T 21N-R 53E-NE NE 11.) go directly from valley fill into rocks of Devonian age without the 'presence of the Garden Valley Formation above the Devonian. However, the presence of the Permian Garden Valley Formation to the west constitutes additional evidence of an eastern source in that the Garden Valley Formation would have to be absent if the source was immediately to the west. 80 The eastern source is inferred to have been located at the present-day site of Diamond Valley. The allochthonous package was probably transported less than 10 miles to its present position. This relatively short distance of transport might also explain the inclusion of the Sadler Ranch Formation in the allochthonous package. The Sadler Ranch is present to the north of the map area and was probably present to the east. The allochthonous rocks were later again displaced by the Tertiary normal faults. Tertiary Normal Faults Normal faults of Tertiary age have served to control the present-day topography of the area. Moreover, the present-day attitude of the low-angle fault plane and the distribution of the allochthonous blocks are also related to the Tertiary faulting. This structural event caused the dismemberment of the K obeh and Old Whalen units and exposed the Hanson Creek and Lone Mountain Dolomite units in the south (see Plate 2, section B-13'). 81 CONCLUSIONS The Ordovician through Middle Devonian rocks mapped in the southern Sulphur Spting,,range were deposited as shallow water sediments in a westward thickening wedge, the Cordilleran geosyncline. This pattern of sedimentation changed with the Late Devonian Antler orogeny. The Hanson Creek Formation was probably deposited in a lagoon during the latest Ordovician. Overlying the Hanson Creek Formation, with a gradational contact, is the lower member of the Lone Mountain Dolomite. The lower member of the Lone Mountain Dolomite is a secondary dolomite that has been interpreted to be a reef complex. The Old Whalen Member of the Lone Mountain Dolomite is the unit with the greatist areal extent in the map area. The Lower Devonian Old Whalen Member represents a repetition of recurring shallow marine environments on a broad carbonate platform. Overlying the Old Whalen Member is the Kobeh Member of the McCalley Canyon Formation. Deposition occured on a shallow shelf under normal marine conditions during the early Pragian. Overlying the Kobeh Member is the abundantly fossiliferous lower part of the Bartine Member of the 82 Mc Calley Canyon Formation. The initial deposits of the lower part of the Bartine were laid down in the latest Pragian-earliest Emsian on a shallow shelf under normal marine conditions, but in deeper water than the Kcbeh Member. The upper part of the Kobeh, found as a single outcrop, is sparsely to moderately fossiliferous. The upper part of the Bartine Member was deposited in the late Emsian and in deeper water than was the lower part. The Sadler Ranch Formation is the first of the allochthonous units found in the map area. The oinoirlal dolomites of the Sad er Ranch Formation were deposited in the late Early Devonian on a shallow shelf in shallow water with open circulation. The second allochthonous unit mapped is the Oxyoke Canyon Sandstone. The peloidal limestones, and quartzites of the lower member of the Oxyoke Canyon Sandstone were deposited in a high to moderate energy lagoon. A change in the depositional energy in the lagoon resulted in the deposition of the dolomitic mudstones of the upper member of the Oxyoke Canyon Sandstones. The Sentinel Mountain Dolomite is the third allochthonous unit found in the study area. The Middle Devonian Sentinel Mountain Dolomite was deposited in a lagoon that initially had open circulation which was later, at least partially, cut off. 83 The Permian Garden Valley Formation is the fourth allochthonous unit found in the map area. The silicified conglomerates of the Garden Valley Formation were deposited as a result of the highland developed during the Antler Orogeny shedding sediments into an adjacent foreland basin. The significance of the Sadler Ranch Formation, Oxyoke Canyon Sandstone, and Sentinel Mountain Dolomite is their stratigraphic position, i.e. the juxtaposition of these units over the Lower Devonian units. The complex stratigraphy of the post-Bartine units led to the discovery of low-angle normal faults, which juxtaposed the Sarller Ranch Formation, Oxyoke Canyon Sandstone, and Sentinel mountain Dolomite rocks over the Old Whalen Member and M c C alley Canyon Formation. The low-angle normal faults also caused the partial to complete denudation of the Kobeh and Bartine Members, and the emplacment of the Permian Garden Valley Formation rocks along the west side of the map area. The key factor in verifying the lithologic evidence was the ages obtained for the various rock units, utilizing conodonts. The dates obtained from the conodonts placed the units within known time frames from which the stratigraphy was worked out. The stratigraphic succession was vital to the discovery of the low-angle normal faults. 84 REFERENCES Armstrong, R. L., 1968, Sevier orogenic belt in Nevada and Utah: GeoL Soc. America Bull., v. 79, p. 427-458. , 1972, Low-angle (denudation) faults, hinterland of the Sevier orogenic belt, eastern Nevada and western Utah: GeoL Soc. America Bull., v. 83, p. 1729-1754. Carlisle, Donald, Murphy, M. A., Nelson, C. A., and Winterer, E. L., 1957, Devonian stratigrphy of Sulphur Spring and Pinyon Ranges, Nevada: Am. Assoc. Petroleum Geologists Bull., v. 41, p. 2175-2191. Colman, R. L., 1979, The carbonate petrology and conodont biostratigtaphy of the Old Whalen Member of the Lone Mountain Dolomite (Lower Devonian), Sulphur Spring Range, Nevada: unpublished M. S. thesis, University of California, Riverside, California, 116 p. Coney, P. J., 1974, Sructural analysis of the Snake Range decollernent, east-central Nevada: GeoL Soc. America BulL, v. 85, p. 973-978. Dunham, J. B., 1977, Depositional environments and paleogeography of the Upper Ordovician, Lower Silurian carbonate platform of central Nevada, in Stewart, J. H., Stevens, C. H., and Fritsche, A. E., eds., Paleozoic paleogeography of the western United States: Soc. Econ. Paleontologists and Mineralogists, Pacific Section, Pacific Coast Paleogeography Symposium 1, p. 157-164. Dunham, R. J., 1962, Classification of carbonate rocks according to depositional texture, in Classification of carbonate rocks, a symposium: Am. Assoc. Petroleum Geologists Mem. 1, p. 108-121. Folk, R. L., 1965, Some aspects of reczystallization in ancient limestones, in Dolomitization and limestone diagenesis-A symposium: Soc. Econ. Paleontologists and Mineralogists Spec. Pub. 13, p. 14-48. 85 Gronberg, E. C., 1967, Stratigraphy of the Nevada Group at Lone Mountain and Tal-ilp Mountain, central Nevada: unpublished M. S. thesis, Unversity of California, Riverside, California, 83 p. Hague, Arnold, 1892, Geology of the Eureka district, Nevada: U. S. GeoL Survey Mon. 20. 419 p. Hose, R. K., and Blake, M. C., 1976, Geology, Pt. I, in Geology and mineral resources of White Pine County, Nevada: Nevada Bur. Mines and Geology BulL 85, p. 1-32. Hose, R. K., Armstrong, A. K., Harris, A. G., and Mamet, B. L., 1982, Devonian and Mimissippian rocks of the northern Antelope Range, Eureka County, Nevada: U. S. Geol Survey Professional Paper 1182, 19 p. Johnson, J. G., 1962, Lower Devonian-Middle Devonian boundary in central Nevada: Am. Assoc. Petroleum Geologists BulL, v. 46., p. 542-546. , 1977, Lower and Middle Devonian faunal intervals in central Nevada based on brachiopods, in Murphy, M. A., Berry, W. B. N., and Sandberg, C. A., eds., Western North America Devonian: University of California, Riverside, Campus Museum Contributions 4, p. 16-32. Johnson, J. G., and Murphy, M. A., 1984, Time-rock model for Siluro-Devonian continental shelf, western United States: Geol. Soc. America BulL, v. 95, p. 1349-1359. Johnson, J. G., and Sandberg, C. A., 1977, Lower and Middle Devonian continental-shelf rocks of the western United States, in Murphy, M. A., Berry, W. B. N., and Sandberg, C. A., eds., Western North America Devonian: University of California, Riverside, Campus Museum Contributions 4, p. 121-143. 86 Kendall, G. W., 1975, Some aspects of Lower and Middle Devonian stratigraphy in Eureka County, Nevada: unpublished M. S. thesis, Oregon State University, Corvallis, Oregon, 199 p. Kendall, G. W., Johnson, J. G., Brown, J. 0., and Klapper, Gilbert, 1983, Stratigraphy and fades acmes Lower Devonian-Middle Devonian boundary, central Nevada: Am. Assoc. Petroleum Geologists Bull., v. 67, p. 2199-2207. Klapper, Gilbert, 1977, Lower and Middle Devonian conodont sequence in central Nevada, with contributions by D. B. Johnson, in Murphy, M. A., Berry, W. B. N., and Sandberg, C. A., eds., Western North America Devonian: University of California, Riverside, Campus Museum Contributions, p. 33-54 Mapper, Gilbert, and Murphy, M. A., 1980, Conodont zonal species from the delta and pesavis Zones (Lower Devonian) in central Nevada: Neues Jahrbuch fur Geologie and Palaontologie Monatsheft, v. 8, p. 490-504. Math, J. C., and McKee, E. H., 1977, Saurian and Lower Devonian paleogeography of the outer continental shelf of the Cordilleran miogeodine, central Nevada, in Stewart, J. H., Stevens, C. H., and Fritsche, A. E., eds., Paleozoic paleogeography of the western United States: Soc. Econ. Paleontologists and Mineralogists, Pacific Section, Pacific Coast Paleogeography Symposium 1, p. 181-215. Merriam, C. W., 1940, Devonian stratigraphy and paleontology of the Roberts Mountains region, Nevada: GeoL Soc. America Spec. Paper 25, 114 p. Mullen, T. E., 1980, Stratigraphy, petrology, and some fossil data of the Roberts Mountains Formation, north-central Nevada: U. S. GeoL Survey Professional Paper 1063, 67 p. 87 Murphy, M. A., and Gronberg, E. C., 1970, Stratigraphy and correlation of the lower Nevada Group (Devonian) north and west of Eureka, Nevada: GeoL Soc. America BulL, v. 81, p. 127-136. Murphy, M. A., Dunham, John, Berry, W. B. N., and Matti, J. C., 1979, Late Llandovery unconformity in central Nevada: Brigham Young University Geology Studies, v. 26, pt.1, p. 21-36. Nichols, K. M., and Saber ling, N. J., 1977, Depositional and tectonic significance of Silurian and Lower Devonian dolomites, Roberts Mountains and vicinity, east-central Nevada, in Stewart, J.H., Stevens, C. H., and Fritsche, A. E., eds., Paleozoic paleogeography of the western United States: Soc. Econ. Paleontologists and Mineralogists, Pacific Section, Pacific Coast Paleogeography Symposium 1, p. 217-240. Nolan, T. B., Merriam, C. W., and Willliams, J. S., 1956, The stratigraphic section in the vicinity of Eureka, Nevada: U. S. Geological Survey Professional Paper 276, 77 p. Roberts, R. J., 1972, Evolution of the Cordilleran fold belt: Geol. Soc. America BulL, v. 83, p. 1989-2004. Roberts, R. J., Montgomery, K. M., and Lehner, R. E., 1967, Geology and mineral resources of Eureka County, Nevada: Nevada Bureau Mines BulL 64, 152 p. Sloss, L. L., 1963, Sequences in the cratonic interior of North America: GeoL Soc. America BulL, v. 74, p. 93-113. Stewart, J. H., 1980, Geology of Nevada: Nevada Bureau of Mines and Geology Spec. Pub. 4, 135 p. Winterer, E. L., and Murphy, M. A., 1960, Silurian reef complex and associated facies, central Nevada: Jour. Geology, v. 68, p. 117-139. APPENDIX 88 APPENDIX FAUNAL LISTS AND LOCALITIES All localities in Garden Valley 15 minute quadrangle. Conodont identification and age aRgignments made by Gilbert Mapper, unit asqignments by J. G. Johnson. Brachiopod identification, age assignment, and not by J. G. Johnson. Coral identification by W m. A. Oliver, Jr.. Conodonts Sample: Location: JL-1 E1Pvation 6000 feet, 600 feet north, S. W. corner Sec.12, T.23 N., R. 52 E.. Pandorinellina expansa Palygnathus serotinus Palygnathus linguifonnis bultyncki? Panderodus sp. Belodell A sp. Age: Unit: Sample: Location: Lower-Middle Devonian, in the range from the serotinus Zone to the costatus Zone. Sadler Ranch Formation. JL-9 Elevation 6040 feet, 1700 feet N., 200 feet S., N. E. corner Sec.14, T. 23 N., R. 52 E.. Icriodus sp. indet. Age: Unit: Devonian Oxyoke Canyon Formation. 89 Sample: Location: JL-34 Elevation 7120 feet, 6500 feet W., 1500 S., S. W. corner Sec. 2, T. 23 N., R. 52 E.. Icriodus Clandi a e Eognathodus sulcatus kindlei Panderodus sp. Age: Unit: Lower Devonian, kindlei Zone. Kobeh Member, McColley Canyon Formation. JL-54 Location: Elevation 6200 feet, 1100 feet E., 300 feet N., S. E. Sample: corner Sec. 11, T. 23 N., R. 52 E.. Palygnathus parawebbi Belodella sp. Age: Unit: Sample: Location: Middle Devonian, australis Zone-Lower varcus Subzone. Sentinel Mountain Dolomite JL-56 Elevation 6520 feet, 7700 feet W., 700 feet N., S. W. corner 7ec. 14, T. 23 N., R. 52 E.. Icriodus sp. indet. Age: Unit: Sample: Location: Lower Devonian, sulcatus Zone to the serotinus Zone. Kobeh Member, McColley Canyon Formation JL-58 Elevation 6800 feet, 8000 feet W., 2100 feet N., S. W. corner Sec. 14, T. 23 N., R. 52 E.. Icriodus trojani Polygnathus sp. indet. Panderodus sp. Belodell Age: Unit: sp. Lower Devonian, dehiscens to serotinus Zones. Bartine Member, McColley Canyon Formation. 90 Sample: Location: JL-63 Elpvation 6520 feet, 3200 feet W., 2700 feet N., S. W. corner Sec. 35, T. 24 N., R. 52 E.. Eognathodus sulcatus kindlei Icriodus sp. indet. Age: Unit: Sample: Location: Lower Devonian, kindlei Zone. Kobeh Member, McColley Canyon Formation. JL-65 Elevation 7240 feet, 5600 feet E., 3900 feet N., S. W. corner Sec. 35, T. 24 N., R. 52 E.. Icriodus claudiae Pandercdus sp. Age: Unit: Sample: Location: Lower Devonian, sulcatus to kindlei Zones. Kobeh Member, McColley Canyon Formation. JL-71 Elevation 7040 feet, 6300 feet W., 900 feet S., S. W. corner Sec. 11, T. 23 N., R. 52 E.. Polygnathus gronbergi Icriodus sp. indet. Pandercdus sp. Age: Unit: Sample: Location: Lower Devonian, gronbergi Zone. Bartine Member, Mc Colley Canyon Formation. JL-74 Elevation 6520 feet., 3000 feet W., 2900 feet S., S. W. corner Sec. 11, T. 23 N., R. 52 E.. Ozarkodina sp. indet. Icriodus sp. indet. Age: Unit: Lower Devonian. Old Whalen Member, Lone Mountain Dolomite. 91 Sample: JL-89 Location: R1Pvation 6160 feet, 300 feet E., 1300 feet S., S. W. corner Sec. 2, T. 23 N., R. 52 E.. Icriodus nevadensis Icriodus trojani Pandorinellina sp. indet. Panderodus sp. Belodella sp. Age: Unit: Sample: Location: Lower Devonian, dehiscens Zone to inverses Zone. Bartine Member, Mc Colley Canyon Formation. JL-90 Plgvation 6240 feet, 500 feet W., 2400 feet S., S. W. corner Sec. 2, T. 23 N., R. 52 E.. Palygnathus n. sp. B Pandorinellina expansa Panderodus sp. Belodella sp. Age: Unit: Sample: Location: Lower Devonian, serotinus Zone to patnbis Zone. Sadler Ranch Formation. JL-95 P.lpvation 6720 feet, 3200 feet W., 2400 feet S, S. W. corner Sec. 2, T. 23 N., R. 52 E.. Icriodus claudiae Age: Unit: Sample: Lower Devonian, sulcatus to kindlei Zones. Kobeh Member, Mc Colley Canyon Formation. JL-96 Location: RiPvation 6520 feet, 7000 feet W., 1000 feet N., S. W. corner Sec. 14, T. 23 N., R. 52 E.. Icriodus claudiae Age: Unit: Lower Devonian, sulc.atus to Icindlei Zones. Kobeh Member, McColley Canyon Formation 92 Sample: Location: JL-116 Elevation 6760 feet, 7300 feet W., 800 feet S., N. W. corner Sec. 23, T. 23 N., R. 52 E.. Icriodus claudiae Age: Unit: Lower Devonian, sulcatus to kindlei Zones. Kobeh Member, Mc Colley Canyon Formation. Sample: JL-119 Location: Elevation 7000 feet, 5100 feet W., 1500 feet N., S. W. Sec. 26, T. 23 N., R. 52 E.. Polygnathus gronbergi Pandorinellina exigua exigua Pandorinellina steinhornensis subsp. inlet. Icriodus nevadensis Icriodus trojani Panderodus sp. Age: Unit: Lower Devonian, gronbergi Zone. Bartine Member, McColl.ey Canyon Formation. Sample: Location: JL-123 Elevation 7200 feet, 5100 feet W., 1500 feet N., S. W. corner Sec. 26, T. 23 N., R. 52 E.. Polygnathus laticostatus Pandatinellina exigua exigua Icriodus trcrjani. Icriodus nevadensis Panderodus sp. Age: Unit: Lower Devonian, inversus Zone. Upper Bartine Member, McCulley Canyon Formation. 93 Sample: Location: JL-129 Elpvation 6080 feet, 2500 feet E., 2400 feet S., S. E. corner Sec. 35, T. 23 N., R. 52 E.. Amorphognathus ordovicicus Pseudobelodina dispansa Drepanaistcdus suberectus Panderodus sp. Age: Ordovician, ordovicicus Zone (Maysvillian to end of Ordovician). Unit: Hanson Creek Formation Brachiopods Sample: Location: JL-71 PlPvation 7040 feet, 6300 feet W., 900 feet S., S. W. oorner Sec. 11, T. 23 N., R. 52 E.. Phragmostrophia merriarni Atrypa nevadana Eurekaspirifer pinyonensis Nucleospira subsphaerica Age: Lower Devonian, Emsian, pinyonensis Zone, Interval 10 or 11. Unit: Bartine Member, Mc Colley Canyon Formation. Sample: JL-73 Elevation 6880 feet, 4200 feet W., 1100 feet S., S. W. corner Sec. 11, T. 23 N., R. 52 E.. Location: Dalejina sp. 3 meristellid indet. 1 Acrospirifer? sp. 3 PLicoplasia cooperi 9 Lower Devonian, Spinoplasia Zone, Interval 5 or 6, based on the Pliooplagia. This Interval occurs in the lowest Kobeh Member rocks in the Sulphur Spring Range and in the Rabbit Hill Limestone to the west, i.e., the Monitor Range. Age: Unit: Kobeh Member, Mc Colley Canyon Formation. 94 Sample: Location: JL-116 Elevation 6760 feet, 7300 feet W., 800 feet S., N. W. corner Sec. 23, T. 23 N., R. 52 E.. Anoplia elongata? 2 Meristella sp. 5 A crospirifex sp. 4 (Sample also contained a spiny platycerid gastropod and rugose coral fragments.) Age: Unit: Lower Devonian, kobehana Zone, Interval 8 or 9. Kobeh Member, M cC alley Canyon Formation. Corals Sample: Location: JL-63 Elevation 6520 feet, 3200 feet W., 2700 feet N., S. W. corner Sec. 35, T. 24 N., R. 52 E.. Emmonsia or Squameofavosites sp Favosites spp. Note: Unit: None of the favositids can be identified from Flory's thesis or the published literature. The specimens of E/S are immature; The F specimens are small fragments. None of the rugosans are identifiable except by knowing their source. All of the listed genera are compatible with the derivation that you indicate. Kobeh M ember, McCulley Canyon Formation.